This story was updated at 11:20 a.m. ET.
Venus is
made of the same stuff of Earth, but is bone-dry, hot enough to melt lead and
has a chokingly thick atmosphere. It even spins backwards.
Astronomers
have spent decades trying to explain Venus' mysterious properties. Now one
scientist thinks the planet's formation may explain all: Two huge, protoplanetary bodies collided head-on and merged
to form our planetary neighbor, but obliterated nearly all water in the process.
"The
probability that two protoplanets collided to form Venus is not at all
implausible," said John Huw Davies, a geodynamicist at Cardiff University in the U.K. who developed the idea.
A majority
of scientists think Earth's moon formed when a protoplanet about the size of
Mars smacked
into the planet at an angle. Davies thinks Venus was born of a far worse cosmic
train wreck.
"What
if the moon-Earth collision isn't that big in planetary terms?" Davies
told SPACE.com. "A head-on blow between two similarly sized bodies
would have been about twice as energetic."
Astronomers
have had little time to react to Davies' proposition, which is detailed in
recent issue of the journal Earth and Planetary Science Letters, but
already some are wary. Despite the cautionary responses from other scientists,
Davies thinks his idea is worth exploring.
Over-baked
Earth
harbors an enormous volume of water, even in its searing interior. The
life-giving molecule emerges as a vapor with molten lava, carrying with it a
radioactive gas known as argon-40. The isotope is generated from radioactive
potassium deposits inside of our planet, as well as in Venus.
Davies
thinks the relatively low amount of such argon detected in Venus'
atmosphere — about 400 times scarcer than on Earth — is a sign that water
never really seeped out of the parched, volcano-covered planet.
"The
only way water could have out-gassed is very early in Venus' history,"
Davies said. "The argon-40 gives us a timescale of water leaving the
ground because it's produced over time, and only a little of it has been
released."
A
mega-collision between two bodies of roughly equal size could have provided the
energy necessary to rip water, which is made of two hydrogen and one oxygen,
into pieces. The hydrogen would escape into space while oxygen would bond with
iron and sink to the planet's core.
Although
the Earth suffered a catastrophic impact that formed the moon, Davies explained
that the process did not dry out the two bodies.
"It
wasn't as energetic, limiting the reaction of iron and water," he said.
Diabolical
deuterium
Tobias
Owens, a planetary scientist at the University of Hawaii, thinks Davies has
"swept deuterium under the rug." This form of hydrogen gas, Owens
explained, can form high in a planet's atmosphere when ultraviolet sunlight
breaks apart a water molecule.
"When
a Venus probe sent back readings of deuterium on the planet, everybody was
astonished," Owens said of a Russian Venus lander mission. "There was
a huge fraction of deuterium 150 times greater than you see on Earth. You have
to explain that."
Owens and
other scientists argue that at 836 degrees F (447 degrees C), Venus' surface
would have instantly baked water into vapor and pushed it into the upper
atmosphere, where sunlight is two times more intense than at Earth. Over time,
he said, the water would degrade.
Davies,
however, said a lack of molecular oxygen — the same type we breathe — produced
by the photo-degradation process does not support such an origin of deuterium.
"Venus
has virtually no oxygen, whereas Earth's atmosphere is about 20 percent
oxygen," Davies said. "If not trapped in the atmosphere, then rocks
would have to absorb it." And evidence from Venus, he said, does not
suggest that this is the case.
Spin
factor
Another clue
that Davies said gives his theory legs is the odd rotation of Venus. The
planet rotates in a clockwise or retrograde direction, which is the
opposite spin of every planet in the inner solar system. "Another peculiarity is
that it has no moon," Davies said. "If the head-on impact I've
hypothesized was a little off of the mark, it could explain Venus' retrograde
rotation without making a moon."
Alan
Boss, a scientist at the Carnegie Institution in Washington, D.C., thinks massive collisions — including head-on mergers — were the norm for terrestrial plants early in their histories and could explain our sinister
twin's backwards habits.
"Venus must have suffered a giant impact during its formation, as did all the terrestrial planets. That is how the final phase of terrestrial planet formation occurs," Boss said in an e-mail. "This could have been a head-on impact, which might not have produced a moon, or it could have been an off-center impact, like the impact that led to Earth's moon."
If the latter was the case, then
where is Venus' moon? Boss explained that if a Venusian moon formed via a giant impact, its orbit could have decayed and spiraled the body into the planet's surface.
Davies
thinks the simpler explanation is his own.
"Of
course it is possible, but it is unclear whether it is probable," Davies
said. Whatever the case, Davies, Boss and most other scientists think big
collision events were common in the solar system's formative years.
New Venusian
visitor?
Aside from planning
to create a detailed computer model for the hypothesized mega-collision, as has
been done for moon formation theory, Davies said another way to test his
idea is to send a new spacecraft to Venus.
Russia's space program successfully landed
nearly 10 spacecraft on Venus' surface in the 1970s and 1980s. But Davies said
none of them scouted for water-containing minerals such as mica — evidence that
would challenge his hypothesis.
"They
made remote chemical measurements of the surface," Davies said, but none
indicated hydrated rocks. "If a new spacecraft finds a lot of hydrated
minerals, it would show there is still abundant water on Venus. Then my
hypothesis would be out."
Spacecraft
that have recently encountered Venus can't detect such minerals from space, he
said, because of a layer of reflective hydrogen sulfide in the
atmosphere.
"A
rover of some sort could scout for such minerals before it fails from the
intense heat, or maybe a satellite below the hydrogen sulfide [layer]," he
said.
Boss,
however, said even detecting such minerals might not rule out a collision.
"Water can always be added as a 'late veneer' by ... icy
planetesimals that helped finish building the planet," Boss said, although
Davies thinks comets and other such bodies could only deliver a small amount of
water to the planet.
Even if hydrated rocks on Venus' surface could rule out a
cataclysmic formation, other data could provide better clues to the planet's
origins, Francis Nimmo of the University of California Santa Cruz thinks.
"There a lot of things that would be very nice to do on
Venus, like put a seismometer on the surface," said Nimmo, a planetary scientist.
"The reason we know anything about Earth's interior is from such
devices."
Whether or not someone launches a new spacecraft to scout
out Venus' surface, and whatever its scientific mission is, Davies said it will
have to investigate quickly.
"You have to take all of your measurements before the
lander, or whatever it is, quite literally burns up," Davies said.
"The longest any spacecraft has lasted is less than two hours."
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